Earth and Planetary Astrophysics (astro-ph.EP)

Abstract: Current space exploration programs call for the establishment of a permanent Human presence on the Moon. This paper considers periodic orbits of a shuttle between the Earth and the Moon. Such a shuttle will be needed to bring supplies to the Moon outpost and carry back those resources that are in short supply on Earth. To keep this shuttle in permanent periodic orbit it must have a thruster that forces it into an elliptical orbit from perigee near Earth to an apogee just beyond the Moon and back to perigee. The impacts of the Earth, Moon and Sun gravity on this orbit are considered. For this model we determine the eccentricity that minimizes the thrust requirements and the lunar $\Delta\, v$ requirements. We show that optimal placements of the eccentricity of the shuttle orbit can produce significant improvement in thrust (and fuel) requirements.

Abstract: On Earth, the development of technology required easy access to open air combustion, which is only possible when oxygen partial pressure, P(O$_2$), is above 18\%. This suggests that only planets with significant atmospheric oxygen concentrations will be capable of developing ``advanced'' technospheres and hence detectable technosignatures.

Abstract: Metal pollution onto white dwarfs is a wide-spread phenomenon that remains puzzling. Some of these white dwarfs also harbour gaseous debris disks. Their emission lines open a unique window to the physical properties of the polluting material, lending insights to their origin. Here, we model the emission line kinematics for the gas disk around SDSS J1228+1040, a system that has been continuously monitored for over two decades. Our model shows that the disk mass is strongly peaked at one solar radius (modulo the unknown inclination), and the disk eccentricity decreases from a value of 0.44 at the disk inner edge, to nearly zero at the outer edge. This eccentricity profile is exactly what one expects if the disk is in a global eccentric mode, precessing rigidly under the combined forces of general relativity and gas pressure, and with a period of 20 yrs. The gas disk contains a mass that is roughly equivalent to that of a 100-km rocky body, while the mass of the accompanying dust disk is likely insignificant. The disk eccentricity confirms an origin in tidal disruption, and we suggest that the disrupted body is sourced from a Mars-mass planetesimal disk within a few AU. More detailed analysis of this disk is warranted.